activity
19942023
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 17.7k across the 141 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

astro-ph2006

Determining the nature of the faint X-ray source population near the Galactic Centre

Reba M. Bandyopadhyay, Andrew J. Gosling, Katherine M. Blundell +5

We present results of a multi-wavelength program to study the faint discrete X-ray source population discovered by Chandra in the Galactic Centre (GC). From IR imaging obtained wit…

astro-ph2006★ 9 cited

Cosmological Implications of the Second Parameter of Type Ia Supernovae

Philipp Podsiadlowski, Paolo A. Mazzali, Pierre Lesaffre +2

Theoretical models predict that the initial metallicity of the progenitor of a Type Ia supernova (SN Ia) affects the peak of the supernova light curve. This can cause a deviation f…

astro-ph2006★ 103 cited

The metallicity dependence of the long-duration GRB rate from host galaxy luminosities

Christian Wolf, Philipp Podsiadlowski

We investigate the difference between the host galaxy properties of core-collapse supernovae and long-duration gamma-ray bursts (LGRBs), and quantify a possible metallicity depende…

astro-ph2006★ 54 cited

The (54Fe+58Ni)/56Ni ratio as a second parameter for Type Ia supernova properties

Paolo A. Mazzali, Philipp Podsiadlowski

A variation of the relative content of (54Fe+58Ni) versus 56Ni may be responsible for the observed scatter of Type Ia Supernovae (SNe Ia) about a mean relation between their intrin…

astro-ph2006★ 91 cited

Double-core evolution and the formation of neutron-star binaries with compact companions

J. D. M. Dewi, Ph. Podsiadlowski, A. Sena

We present the results of a systematic exploration of an alternative evolutionary scenario to form double neutron-star binaries, first proposed by Brown (1995), which does not invo…

astro-ph2006★ 92 cited

A single-degenerate model for the progenitor of the Type Ia supernova 2002ic

Zhanwen Han, Philipp Podsiadlowski

Supernova 2002ic was an atypical Type Ia supernova (SN Ia) with evidence for substantial amounts of hydrogen associated with the system. Contrary to previous claims, we show that i…

astro-ph2006★ 68 cited

The C-flash and the ignition conditions of type Ia supernovae

P. Lesaffre, Z. Han, C. A. Tout +2

Thanks to a stellar evolution code able to compute through the C-flash we link the binary population synthesis of single degenerate progenitors of type Ia supernovae (SNe Ia) to th…

astro-ph2006★ 58 cited

Constraints on SN Ia progenitor time delays from high-z SNe and the star formation history

F. Förster, C. Wolf, Ph. Podsiadlowski +1

We re-assess the question of a systematic time delay between the formation of the progenitor and its explosion in a type Ia supernova (SN Ia) using the Hubble Higher-z Supernova Se…